scholarly journals Reduced model prediction of electron temperature profiles in microtearing-dominated National Spherical Torus eXperiment plasmas

2014 ◽  
Vol 21 (8) ◽  
pp. 082510 ◽  
Author(s):  
S. M. Kaye ◽  
W. Guttenfelder ◽  
R. E. Bell ◽  
S. P. Gerhardt ◽  
B. P. LeBlanc ◽  
...  
Keyword(s):  
Electron Temperature ◽  
Model Prediction ◽  
Reduced Model ◽  
Temperature Profiles ◽  
Spherical Torus

scholarly journals Study of turbulent fluctuations driven by the electron temperature gradient in the National Spherical Torus Experiment

2009 ◽  
Vol 49 (5) ◽  
pp. 055001 ◽  
Author(s):  
E. Mazzucato ◽  
R.E. Bell ◽  
S. Ethier ◽  
J.C. Hosea ◽  
S.M. Kaye ◽  
...  
Keyword(s):  
Temperature Gradient ◽  
Electron Temperature ◽  
Spherical Torus ◽  
Turbulent Fluctuations ◽  
Electron Temperature Gradient

Marginal-Stability Calculation of Electron Temperature Profiles in Tokamaks

1976 ◽  
Vol 37 (5) ◽  
pp. 286-289 ◽  
Author(s):  
Wallace M. Manheimer ◽  
K. R. Chu ◽  
Edward Ott ◽  
Jay P. Boris
Keyword(s):  
Electron Temperature ◽  
Marginal Stability ◽  
Temperature Profiles ◽  
Stability Calculation

Comparison of plasma-density and electron-temperature profiles during the auroral modelling campaign ARIES

1991 ◽  
Vol 69 (8-9) ◽  
pp. 950-958 ◽  
Author(s):  
Joëlle Margot ◽  
A. G. McNamara
Keyword(s):  
Electron Temperature ◽  
Plasma Density ◽  
High Energy ◽  
Primary Electron ◽  
Temperature Profiles ◽  
Height Distribution ◽  
Optical Intensity ◽  
High Energy Electron ◽  
E Region ◽  
Primary Electrons

Plasma-density and electron-temperature profiles were measured during the auroral modelling campaign ARIES. This campaign consisted of two rockets launched in the auroral E region under different geophysical conditions. The plasma-density and electron-temperature behaviours were tentatively related to the energy and intensity of the ionizing primary-electron fluxes. It is concluded that the plasma-density height distribution can be used to estimate the primary-electrons energy. The set of data presented is sufficiently complete to allow, when used together with other types of experiments such as the height distribution of the optical intensity and the high-energy electron spectra, the achievement of the objective of the ARIES multi-instrument campaign, i.e., refinement of the auroral model.

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